Document Type
Article
Abstract
Quantum corrections to Lorentz- and C P T -violating QED in flat spacetime produce unusual radiative corrections, which can be finite but of undetermined magnitude. The corresponding radiative corrections in a gravitational theory are even stranger, since the term in the fermion action involving a preferred axial vector b μ would give rise to a gravitational Chern-Simons term that is proportional b μ , yet which actually does not break Lorentz invariance. Initially, the coefficient of this gravitational Chern-Simons term appears to have the same ambiguity as the coefficient for the analogous term in QED. However, this puzzle is resolved by the fact that the gravitational theory has more stringent gauge invariance requirements. Lorentz symmetry in a metric theory of gravity can only be broken spontaneously, and when the vector b μ arises from spontaneous symmetry breaking, these specific radiative corrections are no longer ambiguous but instead must vanish identically.
Publication Info
Published in Physical Review D, Volume 99, Issue 12, 2019, pages 125009-1-125009-11.
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Altschul, B. (2019). There is no ambiguity in the radiatively induced gravitational Chern-Simons term. Physical Review D, 99(12), 125009. https://doi.org/10.1103/PhysRevD.99.125009
Rights
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Altschul, B. (2019). There is no ambiguity in the radiatively induced gravitational Chern-Simons term. Physical Review D, 99(12), 125009. https://doi.org/10.1103/PhysRevD.99.125009